Dependence of the magnetohydrodynamic shock thickness on the finite electrical conductivity (2004)
- Autores:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- DOI: 10.1017/s0022377803002630
- Assunto: EVOLUÇÃO ESTELAR
- Idioma: Inglês
- Imprenta:
- Fonte:
- Título do periódico: Journal of Plasma Physiscs
- ISSN: 0022-3778
- Volume/Número/Paginação/Ano: v. 79, p. 215-223, 2004
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
KANDUS, Alejandra e OPHER, Reuven. Dependence of the magnetohydrodynamic shock thickness on the finite electrical conductivity. Journal of Plasma Physiscs, v. 79, p. 215-223, 2004Tradução . . Disponível em: https://doi.org/10.1017/s0022377803002630. Acesso em: 19 set. 2024. -
APA
Kandus, A., & Opher, R. (2004). Dependence of the magnetohydrodynamic shock thickness on the finite electrical conductivity. Journal of Plasma Physiscs, 79, 215-223. doi:10.1017/s0022377803002630 -
NLM
Kandus A, Opher R. Dependence of the magnetohydrodynamic shock thickness on the finite electrical conductivity [Internet]. Journal of Plasma Physiscs. 2004 ; 79 215-223.[citado 2024 set. 19 ] Available from: https://doi.org/10.1017/s0022377803002630 -
Vancouver
Kandus A, Opher R. Dependence of the magnetohydrodynamic shock thickness on the finite electrical conductivity [Internet]. Journal of Plasma Physiscs. 2004 ; 79 215-223.[citado 2024 set. 19 ] Available from: https://doi.org/10.1017/s0022377803002630 - Producing superhearvy dark matter during inflation
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Informações sobre o DOI: 10.1017/s0022377803002630 (Fonte: oaDOI API)
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